M. Curé

2.3k total citations
104 papers, 1.2k citations indexed

About

M. Curé is a scholar working on Astronomy and Astrophysics, Instrumentation and Atmospheric Science. According to data from OpenAlex, M. Curé has authored 104 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 57 papers in Astronomy and Astrophysics, 21 papers in Instrumentation and 10 papers in Atmospheric Science. Recurrent topics in M. Curé's work include Stellar, planetary, and galactic studies (54 papers), Astrophysics and Star Formation Studies (43 papers) and Astronomy and Astrophysical Research (21 papers). M. Curé is often cited by papers focused on Stellar, planetary, and galactic studies (54 papers), Astrophysics and Star Formation Studies (43 papers) and Astronomy and Astrophysical Research (21 papers). M. Curé collaborates with scholars based in Chile, Argentina and United States. M. Curé's co-authors include L. S. Cidale, Diego Rial, Bernard Roussel, J. L. Valatx, S. Kanaan, Julio C. Maŕın, M. Kraus, Bernard Rousset, S. Hubrig and M. A. Pogodin and has published in prestigious journals such as PLoS ONE, The Astrophysical Journal and Brain Research.

In The Last Decade

M. Curé

92 papers receiving 1.1k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
M. Curé Chile 21 760 228 97 70 69 104 1.2k
O. Richard France 30 1.4k 1.8× 547 2.4× 61 0.6× 22 0.3× 25 0.4× 139 2.6k
Louis N. Irwin United States 21 576 0.8× 22 0.1× 159 1.6× 35 0.5× 122 1.8× 79 1.4k
D. M. Wilson United States 21 230 0.3× 66 0.3× 19 0.2× 16 0.2× 40 0.6× 40 1.1k
Satoshi Ohashi Japan 23 392 0.5× 14 0.1× 70 0.7× 21 0.3× 97 1.4× 86 1.6k
Marco Bocchio France 17 687 0.9× 87 0.4× 34 0.4× 45 0.6× 79 1.1× 25 1.4k
D. S. Bertram United Kingdom 17 218 0.3× 54 0.2× 67 0.7× 110 1.6× 8 0.1× 57 1.1k
Edward L. Robinson United States 24 787 1.0× 70 0.3× 58 0.6× 48 0.7× 6 0.1× 68 1.4k
Nicholas J. Scott United States 16 519 0.7× 181 0.8× 9 0.1× 7 0.1× 59 0.9× 53 1.0k
Szabolcs Márka United States 23 1.6k 2.1× 29 0.1× 50 0.5× 16 0.2× 13 0.2× 86 2.3k
G. Bono Italy 38 4.5k 6.0× 2.2k 9.7× 33 0.3× 7 0.1× 65 0.9× 214 4.9k

Countries citing papers authored by M. Curé

Since Specialization
Citations

This map shows the geographic impact of M. Curé's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by M. Curé with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Curé more than expected).

Fields of papers citing papers by M. Curé

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. Curé. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by M. Curé. The network helps show where M. Curé may publish in the future.

Co-authorship network of co-authors of M. Curé

This figure shows the co-authorship network connecting the top 25 collaborators of M. Curé. A scholar is included among the top collaborators of M. Curé based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with M. Curé. M. Curé is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Curé, M., et al.. (2025). Unveiling stellar spin: Determining inclination angles in Be stars. Astronomy and Astrophysics. 695. A129–A129.
2.
Curé, M., et al.. (2024). Estimation of Physical Stellar Parameters from Spectral Models Using Deep Learning Techniques. Mathematics. 12(20). 3169–3169. 1 indexed citations
3.
Maŕın, Julio C., et al.. (2023). Forecasting the precipitable water vapour along lines of sight in the Chajnantor region from a WRF simulation. Monthly Notices of the Royal Astronomical Society. 522(1). 457–465.
4.
Carciofi, A. C., P. Santos, R. G. Vieira, et al.. (2023). Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of α Eri and β CMi. Monthly Notices of the Royal Astronomical Society. 526(2). 3007–3036. 13 indexed citations
5.
Cuadra, Jorge, et al.. (2023). Evolution of rotating massive stars with new hydrodynamic wind models. Astronomy and Astrophysics. 673. A109–A109. 8 indexed citations
6.
Curé, M., et al.. (2022). New self-consistent wind parameters to fit optical spectra of O-type stars observed with the HERMES spectrograph. Astronomy and Astrophysics. 661. A51–A51. 9 indexed citations
7.
Fábregas, Ernesto, et al.. (2022). Deep learning exoplanets detection by combining real and synthetic data. PLoS ONE. 17(5). e0268199–e0268199. 6 indexed citations
8.
Curé, M., et al.. (2021). ISOSCELES: Grid of stellar atmosphere and hydrodynamic models of massive stars. The first results. Proceedings of the International Astronomical Union. 17(S370). 180–184. 2 indexed citations
9.
Kanaan, S., et al.. (2018). Spectro-interferometric observations of a sample of Be stars. Astronomy and Astrophysics. 621. A123–A123. 17 indexed citations
10.
Cidale, L. S., et al.. (2018). Wind properties of variable B supergiants. Astronomy and Astrophysics. 614. A91–A91. 32 indexed citations
11.
Kraus, Stefan, J. Kluska, John D. Monnier, et al.. (2018). Imaging the disc rim and a moving close-in companion candidate in the pre-transitional disc of V1247 Orionis. Astronomy and Astrophysics. 621. A7–A7. 6 indexed citations
12.
Klement, Robert, A. C. Carciofi, Th. Rivinius, et al.. (2015). Multitechnique testing of the viscous decretion disk model. Astronomy and Astrophysics. 584. A85–A85. 28 indexed citations
13.
Curé, M., et al.. (2014). A method to deconvolve mass ratio distribution of binary stars. Springer Link (Chiba Institute of Technology). 6 indexed citations
14.
Maŕın, Julio C., et al.. (2013). Dynamics of Local Circulations in Mountainous Terrain during the RHUBC-II Project. Monthly Weather Review. 141(10). 3641–3656. 11 indexed citations
15.
Curé, M., et al.. (2011). VALIDATION OF THE VERTICAL PROFILES OF THREE METEOROLOGICAL MODELS USING RADIOSONDES FROM ANTOFAGASTA, PARANAL AND LLANO DE CHAJNANTOR. Redalyc (Universidad Autónoma del Estado de México). 41. 64–67. 2 indexed citations
16.
Hubrig, S., Markus Schöller, M. Briquet, et al.. (2009). Studying the Magnetic Properties of Upper Main-sequence Stars with FORS1. Open Repository and Bibliography (University of Liège). 135. 21–25. 1 indexed citations
17.
Curé, M.. (2009). Do Hummingbirds See in Ultraviolet?. PubMed. 3(1). 9–12. 2 indexed citations
18.
Hubrig, S., B. Stelzer, M. Schöller, et al.. (2009). Searching for a link between the magnetic nature and other observed properties of Herbig Ae/Bestars and stars with debris disks. Springer Link (Chiba Institute of Technology). 63 indexed citations
19.
Curé, M., et al.. (2006). MODELACIÓN DE LA DISPERSIÓN DE ANHÍDRIDO SULFUROSO EN LA COMUNA DE LA COMUNA DE PUCHUNCAVÍ UTILIZANDO EL PROGRAMA ISC3. Ingeniare. Revista chilena de ingeniería. 14(3). 1 indexed citations
20.
Curé, M., Diego Rial, & L. S. Cidale. (2005). Outflowing disk formation in B supergiants due to rotation and bi-stability in radiation driven winds. El Servicio de Difusión de la Creación Intelectual (National University of La Plata). 26 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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